What is the Divergence of a Point Charge in Cartesian Coordinates?

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SUMMARY

The divergence of a point charge in Cartesian coordinates is not zero, contrasting with the divergence in spherical coordinates, which is zero everywhere except at the origin. The electric field in Cartesian coordinates is expressed as \vec{E} = \frac{q}{4\pi \epsilon_0} \frac{ x \hat{x} + y \hat{y} }{(x^2+y^2)^{\frac{3}{2}}}, leading to a divergence proportional to \nabla \cdot \vec{E} \propto \frac{-2}{(x^2 + y^2)^3}. This discrepancy arises because the spherical coordinate system accounts for the three-dimensional nature of the electric field, while the Cartesian approach restricts it to a plane. The discussion highlights the importance of using the correct coordinate system when analyzing electric fields and their divergences.

PREREQUISITES
  • Understanding of Gauss's Law in electromagnetism
  • Familiarity with vector calculus, specifically divergence
  • Knowledge of electric field representations in both spherical and Cartesian coordinates
  • Basic concepts of charge density and point charges
NEXT STEPS
  • Study the derivation of divergence in spherical coordinates
  • Learn about the implications of charge density in different coordinate systems
  • Explore Griffiths' treatment of electric fields and divergences in "Introduction to Electrodynamics"
  • Investigate the behavior of electric fields in cylindrical coordinates for further comparison
USEFUL FOR

Students and professionals in physics, particularly those focusing on electromagnetism, as well as anyone studying vector calculus and its applications in electric field analysis.

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So I am playing around with the differential form of Gauss's Law:

\nabla \cdot \vec{E} = \frac{\rho}{\epsilon_0}

Starting off simple with a point charge, the electric field is:

\vec{E} = \frac{1}{4 \pi \epsilon_0} \frac{q}{r^2} \hat{r}

And the divergence, in spherical coordinates, is:

\nabla \cdot \vec{E} = \frac{1}{r^2} \frac{\partial}{\partial r} (r^2 E_r)

= \frac{1}{r^2} \frac{\partial}{\partial r} \left( \frac{1}{4 \pi \epsilon_0} \frac{q}{r^2} \right)

= \frac{1}{r^2} \frac{\partial}{\partial r} \left( \frac{q}{4 \pi \epsilon_0}} \right)

= 0

I can handle this much. It makes sense that the divergence is everywhere 0, since the only charge density is a point charge. Griffiths has a discussion about this very thing, where he states that the infinite divergence at the origin causes things to work out as expected.

My problem is in dealing with a cartesian coordinate system. I didn't recall the divergence equation in spherical coordinates when I was first playing around with this, so I tried it in cartesian. Here:

\vec{E} = \frac{q}{4\pi \epsilon_0} \frac{ x \hat{x} + y \hat{y} }{(x^2+y^2)^{\frac{3}{2}}}

But the divergence of this is proportional to:

\nabla \cdot \vec{E} \propto \frac{-2}{(x^2 + y^2)^3}

Which clearly isn't zero everywhere. I've checked my divergence and electric field equation, but I can't find the difference between it and the spherical ones I am using.

So, what gives? Is the divergence in spherical coordinates 0, but nonzero in cartesian?
 
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Isn't there a z axis in Cartesian coordinates? Add this and double check your divergence calculations. :smile:
 
Oh, yes, that would be it. I suppose the equations don't like it very much when you try to restrict the electric field from a point charge to a plane... :redface:

Thanks!
 

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